Chapter 3
Accelerated Many-Core GPU Computing for Physics and Astrophysics on Three Continents
Rainer Spurzem
National Astronomical Observatories of China, Chinese Academy of Sciences, Beijing, China,
Astronomisches Rechen-Institut, Zentrum für Astronomie, University of Heidelberg, Heidelberg, Germany, and
Kavli Institute for Astronomy and Astrophysics, Peking University, Beijing, China
Peter Berczik
National Astronomical Observatories of China, Chinese Academy of Sciences, Beijing, China, and
Astronomisches Rechen-Institut, Zentrum für Astronomie, University of Heidelberg, Heidelberg, Germany
Ingo Berentzen
Zentrum für Astronomie, University of Heidelberg, Heidelberg, Germany
Wei Ge and Xiaowei Wang
Institute of Process Engineering, Chinese Academy of Sciences, Beijing, China
Hsi-Yu Schive
Department of Physics, National Taiwan University, Taibei, Taiwan
Keigo Nitadori
RIKEN AICS Institute, Kobe, Japan
Tsuyoshi Hamada
Nagasaki Advanced Computing Center, Nagasaki University, Nagasaki, Japan
José Fiestas
Astronomisches Rechen-Institut, Zentrum für Astronomie,
University of Heidelberg, Heidelberg, Germany
Theoretical numerical modeling has become a third pillar of sciences in addition to theory and experiment (in the case of astrophysics, the experiment is mostly substituted by observations). Numerical modeling allows one to compare theory with experimental or observational data in unprecedented detail, and it also provides theoretical insight into physical processes ...